Towards the formation problem of dense stellar systems

Details Towards the formation problem of dense stellar systems Towards the formation problem of dense stellar systems

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13..379n&link_type=abstract

In: Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 J

Astronomy and Astrophysics

Astronomy

Dense Stellar Systems

Scientific paper

Two possible formation models of dense stellar systems (DSS) are considered. According to one of these models cold initial conditions can stimulate a collapse and bring to the DSS at least in central region of the system. The stability problem of the collapse is also studied. New asymptotic unknown in cosmology is found. In the frame of other model it is revealed the regions on the diagram “virial ratio ÷ rotation parameter” which are connected with the formation of the DSS.

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